Tunable photonic crystal haloscope for high-mass axion searches
arXiv:2205.08885 · doi:10.1103/PhysRevD.107.015012
Abstract
In the search for axion dark matter, the cavity-based haloscope offers the most sensitive approach to the theoretically interesting models in the microwave region. However, experimental searches have been limited to relatively low masses up to a few tens of eV, benefiting from large detection volumes and high quality factors for a given experimental setup. We propose a new cavity design suitable for axion searches in higher mass regions with enhanced performance. The design features a periodic arrangement of dielectric material in a conventional conducting cavity where the resonant frequency is determined by the interspace. This photonic crystal haloscope can make full use of a given volume even at high frequencies while substantially improving the cavity quality factor. An auxetic structure is considered to deploy the array for two-dimensional frequency tuning. We present the characteristics of this haloscope design and demonstrate its feasibility for high-mass axion searches.
7 pages, 9 figures
References in corpus (5)
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Cited by in corpus (7)
- Searching For Dark Matter with Plasma Haloscopes
- Discovering QCD-Coupled Axion Dark Matter with Polarization Haloscopes
- Low Frequency (100-600 MHz) Searches with Axion Cavity Haloscopes
- Development of axion haloscopes for high-mass search at CAPP
- On the Axion Electrodynamics in a two-dimensional slab and the Casimir effect
- Axionic and nonaxionic electrodynamics in plane and circular geometry
- A new class of axion haloscope resonators: the polygonal coaxial cavity